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Search for axioelectric effect of solar axions using BGO scintillating bolometer
- Derbin, AV;
- Gironi, L;
- Nagorny, SS;
- Pattavina, L;
- Beeman, JW;
- Bellini, F;
- Biassoni, M;
- Capelli, S;
- Clemenza, M;
- Drachnev, IS;
- Ferri, E;
- Giachero, A;
- Gotti, C;
- Kayunov, AS;
- Maiano, C;
- Maino, M;
- Muratova, VN;
- Pavan, M;
- Pirro, S;
- Semenov, DA;
- Sisti, M;
- Unzhakov, EV
Published Web Location
https://doi.org/10.1140/epjc/s10052-014-3035-8Abstract
A search for axioelectric absorption of solar axions produced in the p+d→3He+γ(5.5MeV)$$p + d \rightarrow {^3\mathrm {He}}+\gamma (5.5~\mathrm {MeV})$$ reaction has been performed with a BGO detector placed in a low-background setup. A model-independent limit on the combination of axion–nucleon and axion–electron coupling constants has been obtained: |gAe×gAN3|<1.9×10-10$$| g_{Ae}\times g_{AN}^3|< 1.9\times 10^{-10}$$ for 90 % confidence level. The constraint of the axion–electron coupling constant has been obtained for hadronic axion with masses of (0.1–1) MeV: |gAe|≤(0.96-8.2)×10-8$$|g_{Ae}| \le (0.96 - 8.2)\times 10^{-8}$$.
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